In addition, taking into consideration the limiting case that the compact object is rotating at its mass-shedding limit, then constraints on the maximum value of the kerr parameter, the corresponding equatorial radius, and the central energy density are possible. In particular, firstly we employ the relation found in Ref. [1]}
\(\mathcal {K}_{\rm max} = 0.488 + 0.074 \left(\frac{M_{\rm max}}{M_{\odot }}\right),\) 
